Superradiant scattering of orbital angular momentum beams

被引:6
|
作者
Gooding, Cisco [1 ,2 ]
Weinfurtner, Silke [1 ,3 ]
Unruh, William G. [2 ,4 ]
机构
[1] Univ Nottingham, Sch Math Sci, Nottingham NG7 2RD, England
[2] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z1, Canada
[3] Univ Nottingham, Ctr Math & Theoret Phys Quantum Nonequilibrium Sy, Nottingham NG7 2RD, England
[4] Texas A&M, IQSE, Hagler IAS, College Stn, TX 77843 USA
来源
PHYSICAL REVIEW RESEARCH | 2021年 / 3卷 / 02期
基金
英国工程与自然科学研究理事会; 加拿大自然科学与工程研究理事会;
关键词
GENERATION;
D O I
10.1103/PhysRevResearch.3.023242
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We consider the wave-structure coupling between an acoustic orbital angular momentum beam and a rapidly rotating disk, and present a new configuration exhibiting the wave amplification effect known as rotational superradiance. While initially envisioned in terms of the scattering of an incident wave directed perpendicular to an object's rotation axis, we demonstrate in the context of acoustomechanics that superradiant amplification can also occur with a vortex beam directed parallel to the rotation axis. We propose two different experimental routes: one must either work with rotations high enough that the tangential velocity at the outer edge of the disk exceeds the speed of sound, or use evanescent sound waves. We argue that the latter possibility is more promising, and provides the opportunity to probe a previously unexamined parameter regime in the acoustics of rotating porous media.
引用
收藏
页数:10
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